Geometric actions and flat space holography
Dec 17, 2019Citations per year
Abstract: (Springer)
In this paper we perform the Hamiltonian reduction of the action for three- dimensional Einstein gravity with vanishing cosmological constant using the Chern-Simons formulation and Bondi-van der Burg-Metzner-Sachs (BMS) boundary conditions. An equivalent formulation of the boundary action is the geometric action on BMS coad- joint orbits, where the orbit representative is identified as the bulk holonomy. We use this reduced action to compute one-loop contributions to the torus partition function of all BMS descendants of Minkowski spacetime and cosmological solutions in flat space. We then consider Wilson lines in the ISO(2, 1) Chern-Simons theory with endpoints on the boundary, whose reduction to the boundary theory gives a bilocal operator. We use the expectation values and two-point correlation functions of these bilocal operators to compute quantum contributions to the entanglement entropy of a single interval for BMS invariant field theories and BMS3 blocks, respectively. While semi-classically the BMS boundary theory has central charges c = 0 and c = 3/G, we find that quantum corrections in flat space do not renormalize G, but rather lead to a non-zero c.Note:
- 61 pages, v2: typo's fixed and ref's added, v3: added comments and improved discussions. Matches version accepted for publication in JHEP
- Gauge-gravity correspondence
- Chern-Simons Theories
- Field Theories in Lower Dimensions
- Conformal and W Symmetry
- partition function: torus
- cosmological constant: 0
- space-time: Minkowski
- entropy: entanglement
- correction: quantum
- dimension: 3
References(136)
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